Ushbu ishga iqtibos qilgan ishlar

6 ta ish

Ish: Variation of the X‐Ray Bright Point Number over the Solar Activity Cycle

1. Solar Cycle 23 in Coronal Bright Points

   I. Sattarov, Alexei Pevtsov, Nina Karachik +2

   MaqolaSolar and Space Plasma DynamicsSolar Physics20107 iqtibos

   ABIABI:AkademIndex/openalex/2026.other.307310

2. Rotation of Solar Corona from Tracking of Coronal Bright Points

   Nina Karachik, Alexei Pevtsov, I. Sattarov

   MaqolaSolar and Space Plasma DynamicsThe Astrophysical Journal20065 iqtibos

   ABIABI:AkademIndex/openalex/2006.article.000035

3. Hemispheric asymmetry of coronal bright point’s number and area over solar cycles 23–24

   Nina Karachik, E.P. Minenko

   MaqolaSolar and Space Plasma DynamicsMonthly Notices of the Royal Astronomical Society20251 iqtibos

   ABIABI:AkademIndex/openalex/2025.article.000855

4. What SDO tells us about structure and evolution of coronal bright points

   Nina Karachik, E.P. Minenko, I. Sattarov +2

   MaqolaSolar and Space Plasma DynamicsAstronomische Nachrichten20140 iqtibos

   ABIABI:AkademIndex/openalex/2014.article.000207

5. Investigation of the evolution of coronal bright points and magnetic field topology

   E.P. Minenko, Nina Karachik, I. Sattarov +1

   MaqolaSolar and Space Plasma DynamicsAstronomy Letters20140 iqtibos

   ABIABI:AkademIndex/openalex/2014.article.000224

6. Two types of coronal bright points as indicators of global and local dynamo processes

   Nina Karachik

   MaqolaSolar and Space Plasma DynamicsMonthly Notices of the Royal Astronomical Society20250 iqtibos

   ABIABI:AkademIndex/openalex/2025.article.002370